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Measurement of the total active8B solar neutrino flux at the Sudbury Neutrino Observatory with enhanced neutral current sensitivity

  • S. N. Ahmed
  • , A. E. Anthony
  • , E. W. Beier
  • , A. Bellerive
  • , S. D. Biller
  • , J. Boger
  • , M. G. Boulay
  • , M. G. Bowler
  • , T. J. Bowles
  • , S. J. Brice
  • , T. V. Bullard
  • , Y. D. Chan
  • , M. Chen
  • , X. Chen
  • , B. T. Cleveland
  • , G. A. Cox
  • , X. Dai
  • , F. Dalnoki-Veress
  • , P. J. Doe
  • , R. S. Dosanjh
  • G. Doucas, M. R. Dragowsky, C. A. Duba, F. A. Duncan, M. Dunford, J. A. Dunmore, E. D. Earle, S. R. Elliott, H. C. Evans, G. T. Ewan, J. Farine, H. Fergani, F. Fleurot, J. A. Formaggio, M. M. Fowler, K. Frame, B. G. Fulsom, N. Gagnon, K. Graham, D. R. Grant, R. L. Hahn, J. C. Hall, A. L. Hallin, E. D. Hallman, A. S. Hamer, W. B. Handler, C. K. Hargrove, P. J. Harvey, R. Hazama, K. M. Heeger, W. J. Heintzelman, J. Heise, R. L. Helmer, R. J. Hemingway, A. Hime, M. A. Howe, P. Jagam, N. A. Jelley, J. R. Klein, M. S. Kos, A. V. Krumins, T. Kutter, C. C.M. Kyba, H. Labranche, R. Lange, J. Law, I. T. Lawson, K. T. Lesko, J. R. Leslie, I. Levine, S. Luoma, R. MacLellan, S. Majerus, H. B. Mak, J. Maneira, A. D. Marino, N. McCauley, A. B. McDonald, S. McGee, G. McGregor, C. Mifflin, K. K.S. Miknaitis, G. G. Miller, B. A. Moffat, C. W. Nally, B. G. Nickel, A. J. Noble, E. B. Norman, N. S. Oblath, C. E. Okada, R. W. Ollerhead, J. L. Orrell, S. M. Oser, C. Ouellet, S. J.M. Peeters, A. W.P. Poon, B. C. Robertson, R. G.H. Robertson, E. Rollin, S. S.E. Rosendahl, V. L. Rusu, M. H. Schwendener, O. Simard, J. J. Simpson, C. J. Sims, D. Sinclair, P. Skensved, M. W.E. Smith, N. Starinsky, R. G. Stokstad, L. C. Stonehill, R. Tafirout, Y. Takeuchi, G. Tešić, M. Thomson, M. Thorman, R. van Berg, R. G. van de Water, C. J. Virtue, B. L. Wall, D. Waller, C. E. Waltham, H. Wan Chan Tseung, D. L. Wark, N. West, J. B. Wilhelmy, J. F. Wilkerson, J. R. Wilson, J. M. Wouters, M. Yeh, K. Zuber
  • Department of Physics
  • Queen's University
  • Center for Nonlinear Dynamics
  • The University of Texas at Austin
  • University of Pennsylvania School of Arts and Sciences
  • Department of Physics
  • Carleton University
  • Department of Physics
  • University of Oxford
  • Chemistry Department
  • Brookhaven National Laboratory
  • MST-8, Los Alamos National Laboratory
  • Center for Experimental Nuclear Physics and Astrophysics
  • University of Washington
  • Institute for Nuclear and Particle Astrophysics
  • Ernest Orlando Lawrence Berkeley National Laboratory
  • Department of Physics and Astronomy
  • Laurentian University
  • Department of Physics and Astronomy
  • University of British Columbia
  • TRIUMF
  • Physics Department
  • University of Guelph
  • Department of Physics and Astronomy
  • Indiana University South Bend
  • CCLRC Rutherford Appleton Laboratory
  • Department of Physics and Astronomy
  • University of Sussex

Research output: Contribution to journalArticlepeer-review

777 Citations (Scopus)

Abstract

The measurements performed for determining the total active 8B solar neutrino flux at the Sudbury Neutrino Observatory (SNO) were investigated. The measurements were performed without assumptions about the energy dependence of the survival probability. NaCl dissolved in heavy water was used for making the measurements in order to enhance the sensitivity and signature for neutral-current interactions. The hypothesis of maximal mixing at a confidence level equivalent to 5.4σ was found to be inappropriate by the combined results of global solar and neutrino.

Original languageEnglish
Article number181301
Pages (from-to)181301-1-181301-6
JournalPhysical Review Letters
Volume92
Issue number18
DOIs
Publication statusPublished - 7 May 2004
Externally publishedYes

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